G. Barnes

发表

The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: SHARPs – Space-Weather HMI Active Region Patches

J. T. Hoeksema, M. Turmon, Xudong Sun, 2014, 1404.1879.

A COMPARISON OF FLARE FORECASTING METHODS. I. RESULTS FROM THE “ALL-CLEAR” WORKSHOP

D. S. Bloomfield, M. Wheatland, Rami Qahwaji, 2016, 1608.06319.

Implementing a Magnetic Charge Topology Model for Solar Active Regions

G. Barnes, K. Leka, D. Longcope, 2005 .

Photospheric Magnetic Field Properties of Flaring versus Flare-quiet Active Regions. IV. A Statistically Significant Sample

G. Barnes, K. Leka, 2007 .

HELIOSEISMOLOGY OF PRE-EMERGING ACTIVE REGIONS. III. STATISTICAL ANALYSIS

D. Braun, G. Barnes, K. Leka, 2013, 1307.1938.

HELIOSEISMOLOGY OF PRE-EMERGING ACTIVE REGIONS. II. AVERAGE EMERGENCE PROPERTIES

D. Braun, G. Barnes, K. Leka, 2013, 1303.1391.

Photospheric Magnetic Field Properties of Flaring versus Flare-quiet Active Regions. I. Data, General Approach, and Sample Results

K. D. Leka, G. Barnes, K. Leka, 2003 .

Resolving the Azimuthal Ambiguity in Vector Magnetogram Data with the Divergence-Free Condition: Theoretical Examination

G. Barnes, A. Crouch, 2008 .

Nonlinear Force-Free Modeling of Coronal Magnetic Fields. II. Modeling a Filament Arcade and Simulated Chromospheric and Photospheric Vector Fields

Thomas R. Metcalf, Carolus J. Schrijver, Graham Barnes, 2008 .

Resolving the 180° Ambiguity in Solar Vector Magnetic Field Data: Evaluating the Effects of Noise, Spatial Resolution, and Method Assumptions

Thomas R. Metcalf, Yang Liu, Graham Barnes, 2009 .

A CRITICAL ASSESSMENT OF NONLINEAR FORCE-FREE FIELD MODELING OF THE SOLAR CORONA FOR ACTIVE REGION 10953

Carolus J. Schrijver, Markus J. Aschwanden, Graham Barnes, 2009, 0902.1007.

Modeling and Measuring the Flux Reconnected and Ejected by the Two-Ribbon Flare/CME Event on 7 November 2004

J. Qiu, S. Dasso, B. Ravindra, 2007 .

Angular Momentum Transport in Magnetized Stellar Radiative Zones. III. The Solar Light-Element Abundances

P. Charbonneau, G. Barnes, K. Macgregor, 1999 .

Does Nearby Open Flux Affect the Eruptivity of Solar Active Regions?

G. Barnes, M. Derosa, 2018, The Astrophysical Journal.

Determining the Source of Coronal Helicity through Measurements of Braiding and Spin Helicity Fluxes in Active Regions

B. Ravindra, G. Barnes, D. Longcope, 2007 .

Subsurface Vorticity of Flaring versus Flare-Quiet Active Regions

F. Hill, G. Barnes, K. Leka, 2011 .

Large-scale Spatial Cross-calibration of Hinode/SOT-SP and SDO/HMI

David F. Fouhey, Richard E. L. Higgins, T. Gombosi, 2022, The Astrophysical Journal Supplement Series.

Nonlinear Force-free Field Modeling of a Solar Active Region around the Time of a Major Flare and Coronal Mass Ejection

C. J. Schrijver, M. L. DeRosa, M. S. Wheatland, 2007, 0712.0023.

EFFECTS OF PARTITIONING AND EXTRAPOLATION ON THE CONNECTIVITY OF POTENTIAL MAGNETIC FIELDS

G. Barnes, D. Longcope, C. Beveridge, 2008, 0811.1241.

THE ROLE OF MAGNETIC TOPOLOGY IN THE HEATING OF ACTIVE REGION CORONAL LOOPS

L. Golub, K. Korreck, E. DeLuca, 2010, 1009.2070.

The NWRA Classification Infrastructure: Description and Extension to the Discriminant Analysis Flare Forecasting System (DAFFS)

Graham Barnes, K. D. Leka, G. Barnes, 2018, 1802.06864.

Evaluating (and Improving) Estimates of the Solar Radial Magnetic Field Component from Line-of-Sight Magnetograms

G. Barnes, K. Leka, E. Wagner, 2017, 1701.04836.

Gravity Waves in a Magnetized Shear Layer

P. Charbonneau, G. Barnes, K. Macgregor, 1998 .

Properties of Flare-imminent versus Flare-quiet Active Regions from the Chromosphere through the Corona. II. Nonparametric Discriminant Analysis Results from the NWRA Classification Infrastructure (NCI)

K. Dissauer, G. Barnes, K. Leka, 2022, The Astrophysical Journal.

Inferring Currents from the Zeeman Effect at the Solar Surface

G. Barnes, K. Leka, 2018 .

The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: Optimization of the Spectral Line Inversion Code

Y. Liu, A. Norton, G. Barnes, 2014, Solar Physics.

The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: Optimization of the Spectral Line Inversion Code

R. Centeno, J. Schou, J. Schou, 2014, 1403.3677.

On the Relationship between Coronal Magnetic Null Points and Solar Eruptive Events

G. Barnes, 2007 .

Implications of Different Solar Photospheric Flux-transport Models for Global Coronal and Heliospheric Modeling

Shaela I. Jones, C. Arge, M. Cheung, 2023, The Astrophysical Journal.

Fast and Accurate Emulation of the SDO/HMI Stokes Inversion with Uncertainty Quantification

David F. Fouhey, Spiro K. Antiochos, Tamas I. Gombosi, 2021, The Astrophysical Journal.

HELIOSEISMOLOGY OF PRE-EMERGING ACTIVE REGIONS. I. OVERVIEW, DATA, AND TARGET SELECTION CRITERIA

D. Braun, G. Barnes, K. Leka, 2013, 1303.1433.

Evaluating the Performance of Solar Flare Forecasting Methods

K. D. Leka, G. Barnes, K. Leka, 2008 .

An Overview of Existing Algorithms for Resolving the 180° Ambiguity in Vector Magnetic Fields: Quantitative Tests with Synthetic Data

G. A. Gary, Y. Liu, V. Yurchyshyn, 2006 .

Response to “Comment on ‘Resolving the 180° Ambiguity in Solar Vector Magnetic Field Data: Evaluating the Effects of Noise, Spatial Resolution, and Method Assumptions’ ”

G. A. Gary, Y. Liu, G. Barnes, 2011, 1110.2697.

Modeling and Interpreting the Effects of Spatial Resolution on Solar Magnetic Field Maps

G. Barnes, K. Leka, 2011, 1106.5024.

Photospheric Magnetic Field Properties of Flaring versus Flare-quiet Active Regions. III. Magnetic Charge Topology Models

G. Barnes, K. Leka, 2006 .

The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: Overview and Performance

Jesper Schou, Keiji Hayashi, Graham Barnes, 2014, 1404.1881.

A Fixed-point Scheme for the Numerical Construction of Magnetohydrostatic Atmospheres in Three Dimensions

D. Braun, G. Barnes, S. Gilchrist, 2016, Solar physics.

Resolving the Azimuthal Ambiguity in Vector Magnetogram Data with the Divergence-Free Condition: Application to Discrete Data

G. Barnes, K. Leka, A. Crouch, 2009, 0911.0711.

Recent progress on understanding coronal mass ejection/flare onset by a NASA living with a star focused science team

Shaela I. Jones, Yang Liu, M. Cheung, 2023, Advances in Space Research.

A Comparison of Flare Forecasting Methods. III. Systematic Behaviors of Operational Solar Flare Forecasting Systems

Manolis K. Georgoulis, Rami Qahwaji, Kanya Kusano, 2019, The Astrophysical Journal.

Solar Flare Forecasting: a "State of the Field" Report for Researchers

K. D. Leka, G. Barnes, K. Leka, 2013 .

The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: Overview and Performance

M. Turmon, Xudong Sun, J. Schou, 2014, Solar Physics.

Probabilistic forecasting of solar flares from vector magnetogram data

Everlyn A. Schumer, K. D. Leka, G. Barnes, 2007 .

On the Availability of Sufficient Twist in Solar Active Regions to Trigger the Kink Instability

Y. Fan, G. Barnes, K. Leka, 2005 .

ACHIEVING CONSISTENT DOPPLER MEASUREMENTS FROM SDO/HMI VECTOR FIELD INVERSIONS

S. Antiochos, P. Schuck, G. Barnes, 2015, 1511.06500.

A First Look at Magnetic Field Data Products from SDO/HMI

M. Turmon, Xudong Sun, S. Wu, 2012 .

A Comparison of Flare Forecasting Methods. II. Benchmarks, Metrics, and Performance Results for Operational Solar Flare Forecasting Systems

Manolis K. Georgoulis, Rami Qahwaji, Kanya Kusano, 2019, The Astrophysical Journal Supplement Series.

The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: SHARPs – Space-Weather HMI Active Region Patches

M. Turmon, Y. Liu, X. Sun, 2014, Solar Physics.

Solar Flare Forecasting: Present Methods and Challenges

K. D. Leka, Graham Barnes, G. Barnes, 2018 .